Unique triple star system likely ate a fourth star
Astronomers have detected a triple star system that is unlike any seen before. The unusual trio of stars is much more massive and closely squeezed together than a typical triple system, which may be because the stellar triplets used to have a fourth sibling before one of the others gobbled it up. The tertiary star system is known as
TIC 470710327 and was detected by researchers using data from NASA’S Transiting Exoplanet Survey Satellite
(TESS) observatory, currently orbiting Earth. The trio have a hierarchical structure, meaning a pair of binary stars circle one another at the centre of the system while a third star orbits the central pair.
Triple star systems are not that uncommon: as many as ten per cent of star systems in the universe could be tertiary. In September
2021, astronomers detected a single exoplanet orbiting a tertiary system for the first time, suggesting life could potentially exist in these systems if conditions are right. However, TIC 470710327 stands apart from all the other known tertiary systems because
of its size and shape. The stars are much more massive than the typical stars found within a tertiary system, which also means the trio is much more compact because they all exert a stronger gravitational pull than normal. “As far as we know, it is the first of its kind ever detected,” said Alejandro Vigna-gómez, an astrophysicist at the Niels Bohr Institute at the University of Copenhagen in Denmark.
The binary pair of stars at the heart of
TIC 470710327 have a combined mass of around 12 times the Sun’s, and it takes just over one day for the two stars to orbit one another. The larger outer star is even more massive – weighing about as much as 16 Suns – and it orbits the binary pair once every 52 days.
The new system was originally found by a citizen scientist who was combing through the TESS database in search for abnormalities. The star system stood out to the amateur astronomer due to its high luminosity, a consequence of having three stars shining brightly rather than one. However, it wasn’t until researchers later assessed the data that they realised it was a tertiary system. After discovering how massive the stars are, the team then began trying to figure out how the unusual system might have formed.
There are three potential explanations for how TIC 470710327 was created: the first possibility is that the large outer star formed first, and the smaller stars formed later. This is perhaps the most unlikely explanation, as the massive star would have ejected or absorbed the gas needed to form new stars. The second option is that the three stars all formed separately and gradually gravitated to each other until they started orbiting each other. This is also unlikely because the massive outer star would probably have ended up at the centre of the system.
The third explanation is that the system was originally made up of two binary pairs – the one at the centre of the system we see today and another pair orbiting where the more massive outer star currently sits. Researchers suspect that the outer binary pair then underwent a stellar merger to create a single, more massive star.